We study the Kimble-Braunstein continuous-variable quantum teleportation with the quantum channel physically realized in the turbulent atmosphere. In this context, we examine the applicability of different strategies preserving the Gaussian entanglement (Bohmann et al 2016 Phys. Rev. A 94 010302(R)) for improving the fidelity of the coherent-state teleportation. First, we demonstrate that increasing the squeezing parameter characterizing the entangled state is restricted by its optimal value, which we derive for realistic experimentally-verified examples. Further, we consider the technique of adaptive correlations of losses and show its performance for channels with large squeezing parameters. Finally, we investigate the efficiencies of postselection strategies in dependence on the stochastic properties of the channel transmittance.

Quantum teleportation through atmospheric channels

Bohmann M
2019

Abstract

We study the Kimble-Braunstein continuous-variable quantum teleportation with the quantum channel physically realized in the turbulent atmosphere. In this context, we examine the applicability of different strategies preserving the Gaussian entanglement (Bohmann et al 2016 Phys. Rev. A 94 010302(R)) for improving the fidelity of the coherent-state teleportation. First, we demonstrate that increasing the squeezing parameter characterizing the entangled state is restricted by its optimal value, which we derive for realistic experimentally-verified examples. Further, we consider the technique of adaptive correlations of losses and show its performance for channels with large squeezing parameters. Finally, we investigate the efficiencies of postselection strategies in dependence on the stochastic properties of the channel transmittance.
2019
Istituto Nazionale di Ottica - INO
Inglese
94
12
125104
125104
10
http://www.scopus.com/inward/record.url?eid=2-s2.0-85074542718&partnerID=q2rCbXpz
Sì, ma tipo non specificato
atmospheric quantum optics
quantum teleportation
fluctuating losses
free-space channels
The authors are grateful to D Vasylyev for enlightening discussions. This work has been supported by Deutsche Forschungsgemeinschaft through Grant No. VO 501/22-2. AAS also acknowledges support from the Department of Physics and Astronomy of the NAS of Ukraine through the project PK 0118U003535. MB acknowledges financial support by the Leopoldina Fellowship Programme of the German National Academy of Science (LPDS 2019-01).
4
info:eu-repo/semantics/article
262
Hofmann, K; Semenov, A A; Vogel, W; Bohmann, M
01 Contributo su Rivista::01.01 Articolo in rivista
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/408942
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